Table 3
Meteoroid orbits.
| Name | v g | a | e | i | ω | q | T j | Shower |
| (km s-1) | (AU) | (deg) | (deg) | (AU) | ||||
|
|
||||||||
| 20101016_070052 | 16.7 | 2.46 | 0.657 | 16.9 | 232.254 | 0.844 | 3.1 | |
| ± 0.6 | ± 0.22 | ± 0.031 | ± 0.7 | ± 1.643 | ± 0.009 | ± 0.2 | ||
| 20101016_075031 | 24.2 | 0.55 | 0.856 | 47.1 | 174.964 | 0.079 | 9.7 | |
| ± 0.8 | ± 0.00 | ± 0.014 | ± 3.8 | ± 0.459 | ± 0.008 | ± 0.1 | ||
| 20101020_094418 | 42.7 | 18.44 | 0.947 | 71.0 | 197.381 | 0.974 | 0.7 | |
| ± 0.9 | ± 27.09 | ± 0.077 | ± 1.2 | ± 2.247 | ± 0.005 | ± 0.8 | ||
| 20101020_100214 | 38.6 | 1.13 | 0.527 | 75.2 | 69.568 | 0.532 | 4.8 | |
| ± 0.7 | ± 0.06 | ± 0.02 | ± 1.5 | ± 4.852 | ± 0.029 | ± 0.3 | ||
| 20101103_045928 | 34.5 | 1.22 | 0.906 | 27.9 | 149.33 | 0.115 | 4.6 | |
| ± 0.6 | ± 0.07 | ± 0.008 | ± 2.5 | ± 1.811 | ± 0.011 | ± 0.2 | ||
| 20101103_053624 | 65.1 | 10.18 | 0.954 | 163.8 | 92.053 | 0.474 | -0.3 | ORI |
| ± 0.7 | ± 7.75 | ± 0.035 | ± 2.3 | ± 3.325 | ± 0.026 | ± 1.5 | ||
| 20101103_061856 | 29.5 | 2.37 | 0.859 | 2.4 | 295.999 | 0.333 | 2.9 | NTA |
| ± 0.3 | ± 0.21 | ± 0.008 | ± 1.3 | ± 2.228 | ± 0.014 | ± 0.2 | ||
| 20101103_071855 | 69.6 | 48.10 | 0.98 | 149.5 | 188.636 | 0.987 | -0.9 | |
| ± 0.5 | ± 120.57 | ± 0.051 | ± 1.6 | ± 3.369 | ± 0.004 | ± 1.9 | ||
| 20101106_065820 | 68.3 | 3.05 | 0.675 | 166.9 | 178.592 | 0.991 | 0.6 | |
| ± 1.0 | ± 0.80 | ± 0.085 | ± 1.8 | ± 4.438 | ± 0.001 | ± 0.7 | ||
| 20101107_015015 | 24.7 | 1.69 | 0.754 | 4.5 | 110.453 | 0.416 | 3.8 | NTA |
| ± 0.3 | ± 0.09 | ± 0.008 | ± 1.0 | ± 2.205 | ± 0.014 | ± 0.2 | ||
Notes. vg is the geocentric speed of the meteoroids, corrected for zenithal attraction and diurnal aberration. a is the semimajor axis; e the orbital eccentricity; i the inclination; ω the argument of perihelion, q the perihelion distance, and Tj the Tisserand parameter. Three of the meteors are members of meteor showers: this is marked in the last column.
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